AG would like to thank the referee for their comments and suggestions that improved the content of the paper. AG warmly thanks S. Birrer for useful feedback related to the integration of SLITronomy into the Lenstronomy interface, and feedback and ideas on the paper. AG thanks G. Vernardos and M. Millon for insightful discussions. AG thanks X. Ding for providing the pre-processed HST images used for simulated source galaxies [1]}. AG thanks A.J. Shajib for providing the lens models for SLACS lenses [2]}. This program is supported by the Swiss National Science Foundation (SNSF) and by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (COSMICLENS: grant agreement No 787886). This research made use of Lenstronomy [3]}, [4]}, SciPy [5]}, NumPy [6]}, [7]}, Matplotlib [8]}, scikit-image [9]}, Astropy [10]}, [11]} and Jupyter [12]}.
